Recalibration of Luminosity-HI Linewidth Relations and H_0
| dc.creator | Tully, R. Brent | |
| dc.date | 1998-02-03 | |
| dc.date.accessioned | 2026-07-07T02:25:57Z | |
| dc.date.available | 2026-07-07T02:25:57Z | |
| dc.description | A recalibration of the luminosity-linewidth technique is discussed which introduces (i) new cluster calibration data, (ii) new corrections for reddening as a function of inclination, and (iii) a new zero-point calibration using 13 galaxies with distances determined via the cepheid period-luminosity method. It is found that H_0= 82 +/- 16 km/s/Mpc (95% confidence) | |
| dc.description | 7 pages with 3 figures encapsulated in the .ps file | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9802027 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9802027 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12084 | |
| dc.subject | Astrophysics | |
| dc.title | Recalibration of Luminosity-HI Linewidth Relations and H_0 | |
| dc.type | text |